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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Nonstandard Neutrinos 255<br />

kinematical impact of a m<strong>as</strong>s on certain reactions such <strong>as</strong> nuclear decays<br />

of the <strong>for</strong>m (A, Z) → (A, Z + 1) e − ν e where the continuous energy<br />

spectrum of the electrons originally revealed the emission of another<br />

particle that carried away the remainder of the available energy. The<br />

minimum amount of energy taken by the neutrino is the equivalent of<br />

its m<strong>as</strong>s so that the upper endpoint of the electron spectrum is a sensitive<br />

me<strong>as</strong>ure <strong>for</strong> m νe . Actually, the most sensitive probe is the shape<br />

of the electron spectrum just below its endpoint, not the value of the<br />

endpoint itself. The best constraints are b<strong>as</strong>ed on the tritium decay<br />

3 H → 3 He + e − ν e with a maximum amount of kinetic energy <strong>for</strong> the<br />

electron of Q = 18.6 keV. This unusually small Q-value ensures that a<br />

large fraction of the electron counts appear near the endpoint (Boehm<br />

and Vogel 1987; Winter 1991).<br />

In Tab. 7.1 the results from several recent experiments are summarized<br />

which had been motivated by the Moscow claim of 17 eV <<br />

m νe < 40 eV (Boris et al. 1987). This range is clearly incompatible<br />

with the more recent data which, however, find negative m<strong>as</strong>s-squares.<br />

This means that the endpoint spectra tend to be slightly de<strong>for</strong>med<br />

in the opposite direction from what a neutrino m<strong>as</strong>s would do. This<br />

effect is particularly striking and significant <strong>for</strong> the Livermore experiment<br />

where it is nearly impossible to blame it on a statistical fluctuation.<br />

There<strong>for</strong>e, at the present time one cannot escape the conclusion<br />

that this experimental technique suffers from some unrecognized<br />

systematic effect. This problem must be resolved be<strong>for</strong>e it will<br />

become possible to extract a reliable bound on m νe although it appears<br />

unlikely that an m νe in excess of 10 eV could be hidden by what-<br />

Table 7.1. Summary of tritium β decay experiments.<br />

Experiment m 2 ν e<br />

± σ stat ± σ syst Reference<br />

[eV 2 ]<br />

Los Alamos −147 ± 68 ± 41 Robertson et al. (1991)<br />

Tokyo −65 ± 85 ± 65 Kawakami et al. (1991)<br />

Zürich −24 ± 48 ± 61 Holzschuh et al. (1992)<br />

Mainz −39 ± 34 ± 15 Weinheimer et al. (1993)<br />

Livermore −130 ± 20 ± 15 Stoeffl and Decman (1994)<br />

Troitsk −18 ± 6 Belesev et al. (1994) a<br />

a See Otten (1995) <strong>for</strong> a published description.

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